منابع مشابه
Solar Neutrino Oscillations
This is an invited review talk, presented at the International Conference on Non
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The Sun is a source of high energy neutrinos (E ∼ 10 GeV) produced by cosmic ray interactions in the solar atmosphere. We study the impact of three-flavor oscillations (in vacuum and in matter) on solar atmosphere neutrinos, and calculate their observable fluxes at Earth, as well as their event rates in a kilometer-scale detector in water or ice. We find that peculiar three-flavor oscillation e...
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I describe the current status of the solar neutrino problem, summarizing the arguments that its resolution will require new particle physics. The phenomenon of matter-enhanced neutrino oscillations is reviewed. I consider the implications of current experiments – including the SuperKamiokande atmospheric neutrino and LSND measurements – and the need for additional constraints from SNO and other...
متن کاملNeutrino Oscillations and the Solar Neutrino Problem
I describe the current status of the solar neutrino problem, summarizing the arguments that its resolution will require new particle physics. The phenomenon of matter-enhanced neutrino oscillations is reviewed. I consider the implications of current experiments – including the SuperKamiokande atmospheric neutrino and LSND measurements – and the need for additional constraints from SNO and other...
متن کاملSolar Neutrino Data, Solar Model Uncertainties and Neutrino Oscillations
We incorporate all existing solar neutrino flux measurements and take solar model flux uncertainties into account in deriving global fits to parameter space for the MSW and vacuum solutions of the solar neutrino problem. Also Department of Astronomy. Research supported in part by the DOE, the NSF and the TNRLC. Bitnet: KRAUSS@YALEHEP Supported in part by the DOE.
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ژورنال
عنوان ژورنال: Journal of Physics: Conference Series
سال: 2008
ISSN: 1742-6596
DOI: 10.1088/1742-6596/120/5/052039